Solid-state NMR spectra of natural abundance 13C in reaction centers from photosynthetic bacteria Rhodobacter sphaeroides R-26 was measured. When the quinone acceptors were removed and continuous visible illumination of the sample was provided, exceptionally strong nuclear spin polarization was observed in NMR lines with chemical shifts resembling those of the aromatic carbons in bacteriochlorophyll and bacteriopheophytin. The observation of spin polarized 15N nuclei in bacteriochlorophyll and bacteriopheophytin was previously demonstrated with nonspecifically 15N-labeled reaction centers. Both the carbon and the nitrogen NMR studies indicate that the polarization is developed on species that carry unpaired electrons in the early electron transfer steps, including the bacteriochlorophyll dimer donor P860 and probably the bacteriopheophytin acceptor I. Both enhanced-absorptive and emissive polarization were seen in the carbon spectrum; most lines were absorptive but the methine carbons of the porphyrin ring (a, .3, y, 8) exhibited emissive polarization. The change in the sign of the hyperfine coupling at these sites indicates the existence of nodes in the spin density distribution on the tetrapyrrole cofactors flanking each methine carbon bridge.We previously reported that light-induced nuclear spin polarization in the 15N solid-state NMR (SSNMR) spectra of photosynthetic reaction centers made it possible to detect nitrogen nuclei located in the active site of the protein with enormous intensities not attainable under typical experimental conditions (1). These studies were done using nonspecifically labeled reaction centers in which the quinone acceptors were either missing or chemically reduced; the known photochemical cycles of the remaining bacteriochlorophyll and bacteriopheophytin donor and acceptor species make them probable candidates for radical-pair-type chemically induced dynamic nuclear polarization (CIDNP) processes (2). A paper with the chemical assignments for the 15N polarized signals is forthcoming (3). We now report the observation of photo-CIDNP that allows us to detect the SSNMR spectra of natural abundance 13C in quinone-depleted photosynthetic reaction centers from Rhodobacter sphaeroides R-26 (see Fig. 1).The study of large biological systems by SSNMR usually requires specific isotopic labeling with an NMR observable nucleus, which can be burdensome and expensive in some cases and impossible in others. Specific isotopic labeling has been used in the study of photosynthetic reaction centers from R. sphaeroides (4, 5), as well as in other systems of biophysical interest (6). The finding we report is remarkable in the sense that exceptionally large NMR signals from the active site of a large protein are obtained even in the absence of any kind of isotopic enrichment.The reaction center from R. sphaeroides R-26 is a transmembrane protein with a known structure (7), consisting of three subunits (L, M, and H) and nine cofactors (four bacteriochlorophylls, two bacteriopheophytins, two qu...